ProcessCcdWithVariableFakesTask¶
- class lsst.pipe.tasks.processCcdWithFakes.ProcessCcdWithVariableFakesTask(schema=None, butler=None, **kwargs)¶
Bases:
ProcessCcdWithFakesTaskAs ProcessCcdWithFakes except add variablity to the fakes catalog magnitude in the observed band for this ccdVisit.
Additionally, write out the modified magnitudes to the Butler.
Attributes Summary
Methods Summary
addVariability(fakeCat, band, exposure, ...)Add scatter to the fake catalog visit magnitudes.
composeFakeCat(fakeCats, skyMap)Concatenate the fakeCats from tracts that may cover the exposure.
copyCalibrationFields(calibCat, sourceCat, ...)Match sources in calibCat and sourceCat and copy the specified fields
Empty (clear) the metadata for this Task and all sub-Tasks.
Get metadata for all tasks.
Get the task name as a hierarchical name including parent task names.
getName()Get the name of the task.
Get a dictionary of all tasks as a shallow copy.
getVisitMatchedFakeCat(fakeCat, exposure)Trim the fakeCat to select particular visit
makeField(doc)Make a
lsst.pex.config.ConfigurableFieldfor this task.makeSubtask(name, **keyArgs)Create a subtask as a new instance as the
nameattribute of this task.run(fakeCats, exposure, skyMap[, wcs, ...])Add fake sources to a calexp and then run detection, deblending and measurement.
runQuantum(butlerQC, inputRefs, outputRefs)Do butler IO and transform to provide in memory objects for tasks
runmethod.timer(name[, logLevel])Context manager to log performance data for an arbitrary block of code.
Attributes Documentation
Methods Documentation
- addVariability(fakeCat, band, exposure, photoCalib, rngSeed)¶
Add scatter to the fake catalog visit magnitudes.
Currently just adds a simple Gaussian scatter around the static fake magnitude. This function could be modified to return any number of fake variability.
- Parameters:
- fakeCat
pandas.DataFrame Catalog of fakes to modify magnitudes of.
- band
str Current observing band to modify.
- exposure
lsst.afw.image.ExposureF Exposure fakes will be added to.
- photoCalib
lsst.afw.image.PhotoCalib Photometric calibration object of
exposure.- rngSeed
int Random number generator seed.
- fakeCat
- Returns:
- dataFrame
pandas.DataFrame DataFrame containing the values of the magnitudes to that will be inserted into this ccdVisit.
- dataFrame
- composeFakeCat(fakeCats, skyMap)¶
Concatenate the fakeCats from tracts that may cover the exposure.
- Parameters:
- fakeCats
listoflsst.daf.butler.DeferredDatasetHandle Set of fake cats to concatenate.
- skyMap
lsst.skymap.SkyMap SkyMap defining the geometry of the tracts and patches.
- fakeCats
- Returns:
- combinedFakeCat
pandas.DataFrame All fakes that cover the inner polygon of the tracts in this quantum.
- combinedFakeCat
- copyCalibrationFields(calibCat, sourceCat, fieldsToCopy)¶
Match sources in calibCat and sourceCat and copy the specified fields
- Parameters:
- calibCat
lsst.afw.table.SourceCatalog Catalog from which to copy fields.
- sourceCat
lsst.afw.table.SourceCatalog Catalog to which to copy fields.
- fieldsToCopy
lsst.pex.config.listField.List Fields to copy from calibCat to SoourceCat.
- calibCat
- Returns:
- newCat
lsst.afw.table.SourceCatalog Catalog which includes the copied fields.
- The fields copied are those specified by
fieldsToCopythat actually exist - in the schema of
calibCat. - This version was based on and adapted from the one in calibrateTask.
- newCat
- getFullMetadata() TaskMetadata¶
Get metadata for all tasks.
- Returns:
- metadata
TaskMetadata The keys are the full task name. Values are metadata for the top-level task and all subtasks, sub-subtasks, etc.
- metadata
Notes
The returned metadata includes timing information (if
@timer.timeMethodis used) and any metadata set by the task. The name of each item consists of the full task name with.replaced by:, followed by.and the name of the item, e.g.:topLevelTaskName:subtaskName:subsubtaskName.itemName
using
:in the full task name disambiguates the rare situation that a task has a subtask and a metadata item with the same name.
- getFullName() str¶
Get the task name as a hierarchical name including parent task names.
- Returns:
- fullName
str The full name consists of the name of the parent task and each subtask separated by periods. For example:
The full name of top-level task “top” is simply “top”.
The full name of subtask “sub” of top-level task “top” is “top.sub”.
The full name of subtask “sub2” of subtask “sub” of top-level task “top” is “top.sub.sub2”.
- fullName
- getTaskDict() dict[str, weakref.ReferenceType[lsst.pipe.base.task.Task]]¶
Get a dictionary of all tasks as a shallow copy.
- Returns:
- taskDict
dict Dictionary containing full task name: task object for the top-level task and all subtasks, sub-subtasks, etc.
- taskDict
- getVisitMatchedFakeCat(fakeCat, exposure)¶
Trim the fakeCat to select particular visit
- Parameters:
- fakeCat
pandas.core.frame.DataFrame The catalog of fake sources to add to the exposure
- exposure
lsst.afw.image.exposure.exposure.ExposureF The exposure to add the fake sources to
- fakeCat
- Returns:
- movingFakeCat
pandas.DataFrame All fakes that belong to the visit
- movingFakeCat
- classmethod makeField(doc: str) ConfigurableField¶
Make a
lsst.pex.config.ConfigurableFieldfor this task.- Parameters:
- doc
str Help text for the field.
- doc
- Returns:
- configurableField
lsst.pex.config.ConfigurableField A
ConfigurableFieldfor this task.
- configurableField
Examples
Provides a convenient way to specify this task is a subtask of another task.
Here is an example of use:
class OtherTaskConfig(lsst.pex.config.Config): aSubtask = ATaskClass.makeField("brief description of task")
- makeSubtask(name: str, **keyArgs: Any) None¶
Create a subtask as a new instance as the
nameattribute of this task.- Parameters:
- name
str Brief name of the subtask.
- **keyArgs
Extra keyword arguments used to construct the task. The following arguments are automatically provided and cannot be overridden:
config.parentTask.
- name
Notes
The subtask must be defined by
Task.config.name, an instance ofConfigurableFieldorRegistryField.
- run(fakeCats, exposure, skyMap, wcs=None, photoCalib=None, exposureIdInfo=None, icSourceCat=None, sfdSourceCat=None, idGenerator=None)¶
Add fake sources to a calexp and then run detection, deblending and measurement.
- Parameters:
- fakeCat
pandas.core.frame.DataFrame The catalog of fake sources to add to the exposure.
- exposure
lsst.afw.image.exposure.exposure.ExposureF The exposure to add the fake sources to.
- skyMap
lsst.skymap.SkyMap SkyMap defining the tracts and patches the fakes are stored over.
- wcs
lsst.afw.geom.SkyWcs, optional WCS to use to add fake sources.
- photoCalib
lsst.afw.image.photoCalib.PhotoCalib, optional Photometric calibration to be used to calibrate the fake sources.
- exposureIdInfo
lsst.obs.base.ExposureIdInfo, optional Object that carries ID information for this image/catalog. Deprecated in favor of
idGenerator.- icSourceCat
lsst.afw.table.SourceCatalog, optional Catalog to take the information about which sources were used for calibration from.
- sfdSourceCat
lsst.afw.table.SourceCatalog, optional Catalog produced by singleFrameDriver, needed to copy some calibration flags from.
- idGenerator
lsst.meas.base.IdGenerator, optional Object that generates Source IDs and random seeds.
- fakeCat
- Returns:
- resultStruct
lsst.pipe.base.struct.Struct Results struct containing:
outputExposure : Exposure with added fakes (
lsst.afw.image.exposure.exposure.ExposureF)outputCat : Catalog with detected fakes (
lsst.afw.table.source.source.SourceCatalog)ccdVisitFakeMagnitudes : Magnitudes that these fakes were inserted with after being scattered (
pandas.DataFrame)
- resultStruct
Notes
Adds pixel coordinates for each source to the fakeCat and removes objects with bulge or disk half light radius = 0 (if
config.cleanCat = True). These columns are calledxandyand are in pixels.Adds the
Fakemask plane to the exposure which is then set byaddFakeSourcesto mark where fake sources have been added. Uses the information in thefakeCatto make fake galaxies (using galsim) and fake stars, using the PSF models from the PSF information for the calexp. These are then added to the calexp and the calexp with fakes included returned.The galsim galaxies are made using a double sersic profile, one for the bulge and one for the disk, this is then convolved with the PSF at that point.
- runQuantum(butlerQC, inputRefs, outputRefs)¶
Do butler IO and transform to provide in memory objects for tasks
runmethod.- Parameters:
- butlerQC
ButlerQuantumContext A butler which is specialized to operate in the context of a
lsst.daf.butler.Quantum.- inputRefs
InputQuantizedConnection Datastructure whose attribute names are the names that identify connections defined in corresponding
PipelineTaskConnectionsclass. The values of these attributes are thelsst.daf.butler.DatasetRefobjects associated with the defined input/prerequisite connections.- outputRefs
OutputQuantizedConnection Datastructure whose attribute names are the names that identify connections defined in corresponding
PipelineTaskConnectionsclass. The values of these attributes are thelsst.daf.butler.DatasetRefobjects associated with the defined output connections.
- butlerQC